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THE COSMIC MeV GAMMA-RAY BACKGROUND AND HARD X-RAY SPECTRA OF ACTIVE GALACTIC NUCLEI: IMPLICATIONS FOR THE ORIGIN OF HOT AGN CORONAE

机译:活性银河系核的宇宙MeV伽玛射线背景和X射线硬光谱:对热银冠冕起源的启示

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摘要

The origin of the extragalactic gamma-ray background radiation at 1-10 MeV is still unknown. Although the cosmic X-ray background up to a few hundred keV can be accounted for by the sum of active galactic nuclei (AGNs), current models of AGN spectra canno
机译:1-10 MeV的银河外γ射线背景辐射的起源仍然未知。尽管活动银河核(AGN)的总和可以解释高达几百keV的宇宙X射线背景,但当前的AGN光谱模型无法解决

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